Annual parallax measurement of extreme OH/IR candidate star OH39.7+1.5
Annual parallax measurement of extreme OH/IR candidate star OH39.7+1.5
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Publisher
Cambridge, UK: Cambridge University Press
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Language
English
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Publisher
Cambridge, UK: Cambridge University Press
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Contents
OH/IR stars are low- to intermediate-mass stars (about 0.5-8 solar masses) in the AGB phase, and are considered to be in the process of evolving from Mira variables to planetary nebulae. We aim to understand the evolutionary stages of these AGB stars by approaching them from astrometric VLBI observations with VERA. In 2017, we have started VLBI obs...
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Full title
Annual parallax measurement of extreme OH/IR candidate star OH39.7+1.5
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TN_cdi_proquest_journals_2922792530
Permalink
https://devfeature-collection.sl.nsw.gov.au/record/TN_cdi_proquest_journals_2922792530
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ISSN
1743-9213
E-ISSN
1743-9221
DOI
10.1017/S1743921323003137
